... : 相位估计 X射线脉冲星 泊松过程 最大似然估计 Monte-carlo [gap=934]Keywords : Phase estimation; X-ray pulsar; Poisson process; Maximum-likelihood method(ML); Monte Carlo ..
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The luminosity and the energy of emission line correlate with the pulse phase of X-ray pulsar as well.
而且发射线的强度和能量均与脉冲相位关联。
Astronomers using NASA's Chandra X-ray Observatory found that this pulsar, known as PSR J0357+3205 (or PSR J0357 for short), apparently has a long, bright X-ray tail streaming away from it.
天文学家通过美国宇航局(NASA)的钱德拉(Chandra ) X 射线天文台,发现了这个被称作 PSR J0357+3205(或简称为 PSR J0357)的脉冲星。 很明显,它留下了一条长而明亮的 X 射线尾巴。
Besides, the X-ray pulses detected from pulsar B were too strong.
此外,来自脉冲星b的X射线脉冲也很强。
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